Fig. 4.

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Best-fit results for the dust parameters as a function of log(M⋆/M⊙) for the fitted DES galaxies with DECam global (left panels) and local (right panels) griz photometry. Plots for τV are shown in the top row, while results for n are shown in the bottom row. The best-fit for the age of each galaxy is plotted on a gradient from blue (younger) to red (older).
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